BEGIN:VCALENDAR VERSION:2.0 PRODID:-//CERN//INDICO//EN BEGIN:VEVENT SUMMARY:Field Theory\n DTSTART;VALUE=DATE-TIME:19991108T090000Z DTEND;VALUE=DATE-TIME:19991108T130000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032361@cern.ch DESCRIPTION:Lecture 1\nIn these lectures I will build up the concept of fi eld theory using the language of Feynman diagrams. As a starting point\, f ield theory in zero spacetime dimensions is used as a vehicle to develop a ll the necessary techniques: path integral\, Feynman diagrams\, Schwinger- Dyson equations\, asymptotic series\, effective action\, renormalization e tc. The theory is then extended to more dimensions\, with emphasis on the combinatorial aspects of the diagrams rather than their particular mathema tical structure. The concept of unitarity is used to\, finally\, arrive at the various Feynman rules in an actual\, four-dimensional theory. The con cept of gauge-invariance is developed\, and the structure of a non-abelian gauge theory is discussed\, again on the level of Feynman diagrams and Fe ynman rules.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a032361 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032361 END:VEVENT BEGIN:VEVENT SUMMARY:Field Theory\n DTSTART;VALUE=DATE-TIME:19991109T090000Z DTEND;VALUE=DATE-TIME:19991109T091500Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032401@cern.ch DESCRIPTION:Lecture 2\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId =a032401 LOCATION:CERN Council Chamber URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032401 END:VEVENT BEGIN:VEVENT SUMMARY:Field Theory\n DTSTART;VALUE=DATE-TIME:19991110T090000Z DTEND;VALUE=DATE-TIME:19991110T130000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032402@cern.ch DESCRIPTION:Lecture 3\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId =a032402 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032402 END:VEVENT BEGIN:VEVENT SUMMARY:Field Theory\n DTSTART;VALUE=DATE-TIME:19991111T090000Z DTEND;VALUE=DATE-TIME:19991111T100000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032403@cern.ch DESCRIPTION:Lecture 4\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId =a032403 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032403 END:VEVENT BEGIN:VEVENT SUMMARY:Field Theory\n DTSTART;VALUE=DATE-TIME:19991112T090000Z DTEND;VALUE=DATE-TIME:19991112T130000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032404@cern.ch DESCRIPTION:Lecture 5\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId =a032404 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032404 END:VEVENT BEGIN:VEVENT SUMMARY:QCD\n DTSTART;VALUE=DATE-TIME:19991115T100000Z DTEND;VALUE=DATE-TIME:19991115T101500Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032405@cern.ch DESCRIPTION:Lecture 1\nThe lectures will first cover the basic properties of QCD: the Lagrangian\, the running coupling\, asymptotic freedom and col our confinement. Next\, some examples of perturbative calculations in elec tron-positron physics (total cross sections and event shapes) will be give n. The "parton branching" approach will then be used to derive the evoluti on equations for hadron structure functions and jet fragmentation function s.\nComparisons with data on deep inelastic scattering and jet production will be given. Hadronization models will be described and compared with re cent data. If time permits\, non-perturbative corrections to perturbative QCD predictions will be also be discussed.\n\nhttp://indico.cern.ch/confer enceDisplay.py?confId=a032405 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032405 END:VEVENT BEGIN:VEVENT SUMMARY:QCD\n DTSTART;VALUE=DATE-TIME:19991116T100000Z DTEND;VALUE=DATE-TIME:19991116T130000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032406@cern.ch DESCRIPTION:Lecture 2\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId =a032406 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032406 END:VEVENT BEGIN:VEVENT SUMMARY:QCD\n DTSTART;VALUE=DATE-TIME:19991117T100000Z DTEND;VALUE=DATE-TIME:19991117T130000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032407@cern.ch DESCRIPTION:Lecture 3\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId =a032407 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032407 END:VEVENT BEGIN:VEVENT SUMMARY:QCD DTSTART;VALUE=DATE-TIME:19991118T100000Z DTEND;VALUE=DATE-TIME:19991118T130000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032408@cern.ch DESCRIPTION:Lecture 4\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId =a032408 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032408 END:VEVENT BEGIN:VEVENT SUMMARY:QCD DTSTART;VALUE=DATE-TIME:19991119T100000Z DTEND;VALUE=DATE-TIME:19991119T130000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032409@cern.ch DESCRIPTION:Lecture 5\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId =a032409 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032409 END:VEVENT BEGIN:VEVENT SUMMARY:Standard Model Physics\n\n DTSTART;VALUE=DATE-TIME:19991122T100000Z DTEND;VALUE=DATE-TIME:19991122T101500Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032410@cern.ch DESCRIPTION:Lecture 1\nIntroduction. Structure of gauge theories. The QED and QCD examples. Chiral theories. The electroweak theory. Spontaneous sym metry breaking. The Higgs mechanism. Gauge boson and fermion masses. Yukaw a couplings. Charges current couplings. The Cabibbo-Kobayashi-Maskawa matr ix and CP violation. Neutral current couplings. The Glashow-Iliopoulos-Mai ani mechanism. Gauge boson and Higgs couplings. Radiative corrections and loops. Cancellation of the chiral anomaly. Limits on the Higgs mass. Compa rison with experiment. Problems of the \nStandard Model. Outlook.\n\nhttp: //indico.cern.ch/conferenceDisplay.py?confId=a032410 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032410 END:VEVENT BEGIN:VEVENT SUMMARY:Standard Model Physics DTSTART;VALUE=DATE-TIME:19991123T100000Z DTEND;VALUE=DATE-TIME:19991123T130000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032411@cern.ch DESCRIPTION:Lecture 2\nIntroduction. Structure of gauge theories. The QED and QCD examples. Chiral theories. The electroweak theory. Spontaneous sym metry breaking. The Higgs mechanism. Gauge boson and fermion masses. Yukaw a couplings. Charges current couplings. The Cabibbo-Kobayashi-Maskawa matr ix and CP violation. Neutral current couplings. The Glashow-Iliopoulos-Mai ani mechanism. Gauge boson and Higgs couplings. Radiative corrections and loops. Cancellation of the chiral anomaly. Limits on the Higgs mass. Compa rison with experiment. Problems of the \nStandard Model. Outlook.\n\nhttp: //indico.cern.ch/conferenceDisplay.py?confId=a032411 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032411 END:VEVENT BEGIN:VEVENT SUMMARY:Standard Model Physics DTSTART;VALUE=DATE-TIME:19991124T100000Z DTEND;VALUE=DATE-TIME:19991124T130000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032412@cern.ch DESCRIPTION:Lecture 3\nIntroduction. Structure of gauge theories. The QED and QCD examples. Chiral theories. The electroweak theory. Spontaneous sym metry breaking. The Higgs mechanism. Gauge boson and fermion masses. Yukaw a couplings. Charges current couplings. The Cabibbo-Kobayashi-Maskawa matr ix and CP violation. Neutral current couplings. The Glashow-Iliopoulos-Mai ani mechanism. Gauge boson and Higgs couplings. Radiative corrections and loops. Cancellation of the chiral anomaly. Limits on the Higgs mass. Compa rison with experiment. Problems of the \nStandard Model. Outlook.\n\nhttp: //indico.cern.ch/conferenceDisplay.py?confId=a032412 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032412 END:VEVENT BEGIN:VEVENT SUMMARY:Standard Model Physics DTSTART;VALUE=DATE-TIME:19991125T100000Z DTEND;VALUE=DATE-TIME:19991125T130000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032413@cern.ch DESCRIPTION:Lecture 4\nIntroduction. Structure of gauge theories. The QED and QCD examples. Chiral theories. The electroweak theory. Spontaneous sym metry breaking. The Higgs mechanism. Gauge boson and fermion masses. Yukaw a couplings. Charges current couplings. The Cabibbo-Kobayashi-Maskawa matr ix and CP violation. Neutral current couplings. The Glashow-Iliopoulos-Mai ani mechanism. Gauge boson and Higgs couplings. Radiative corrections and loops. Cancellation of the chiral anomaly. Limits on the Higgs mass. Compa rison with experiment. Problems of the \nStandard Model. Outlook.\n\nhttp: //indico.cern.ch/conferenceDisplay.py?confId=a032413 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032413 END:VEVENT BEGIN:VEVENT SUMMARY:Standard Model Physics DTSTART;VALUE=DATE-TIME:19991126T100000Z DTEND;VALUE=DATE-TIME:19991126T130000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032414@cern.ch DESCRIPTION:Lecture 5\nIntroduction. Structure of gauge theories. The QED and QCD examples. Chiral theories. The electroweak theory. Spontaneous sym metry breaking. The Higgs mechanism. Gauge boson and fermion masses. Yukaw a couplings. Charges current couplings. The Cabibbo-Kobayashi-Maskawa matr ix and CP violation. Neutral current couplings. The Glashow-Iliopoulos-Mai ani mechanism. Gauge boson and Higgs couplings. Radiative corrections and loops. Cancellation of the chiral anomaly. Limits on the Higgs mass. Compa rison with experiment. Problems of the \nStandard Model. Outlook.\n\nhttp: //indico.cern.ch/conferenceDisplay.py?confId=a032414 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032414 END:VEVENT BEGIN:VEVENT SUMMARY:Basic Processes and Trends in Gaseous Detectors\n DTSTART;VALUE=DATE-TIME:19991206T100000Z DTEND;VALUE=DATE-TIME:19991206T130000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032415@cern.ch DESCRIPTION:Lecture 1\nAlmost a century after the invention of the proport ional counter\, a large research effort is still devoted to better underst and the basic properties of gaseous detectors\, and to improve their perfo rmances and reliability\, particularly in view of use at the high radiatio n levels expected at LHC. In the first part of the lectures\, after a brie f introduction on underlying physical phenomena\, I will review modern sop histicated computational tools\, as well as some classic 'back \nof the en velope' analytical methods\, available today for estimating the general pe rformances of gaseous detectors. In the second part\, I will analyse in mo re detail problems specific to the use of \ndetectors at high rates (space charge\, discharges\, aging)\, and describe the recent development of pow erful and perhaps more reliable devices\, particularly in the field of pos ition-sensitive micro-pattern detectors.\n\nhttp://indico.cern.ch/conferen ceDisplay.py?confId=a032415 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032415 END:VEVENT BEGIN:VEVENT SUMMARY:Basic Processes and Trends in Gaseous Detectors DTSTART;VALUE=DATE-TIME:19991207T100000Z DTEND;VALUE=DATE-TIME:19991207T130000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032416@cern.ch DESCRIPTION:Lecture 2\nAlmost a century after the invention of the proport ional counter\, a large research effort is still devoted to better underst and the basic properties of gaseous detectors\, and to improve their perfo rmances and reliability\, particularly in view of use at the high radiatio n levels expected at LHC. In the first part of the lectures\, after a brie f introduction on underlying physical phenomena\, I will review modern sop histicated computational tools\, as well as some classic 'back \nof the en velope' analytical methods\, available today for estimating the general pe rformances of gaseous detectors. In the second part\, I will analyse in mo re detail problems specific to the use of detectors at high rates (space c harge\, discharges\, aging)\, and describe the recent development of power ful and perhaps more reliable devices\, particularly in the field of posit ion-sensitive micro-pattern detectors.\n\nhttp://indico.cern.ch/conference Display.py?confId=a032416 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032416 END:VEVENT BEGIN:VEVENT SUMMARY:Basic Processes and Trends in Gaseous Detectors\n DTSTART;VALUE=DATE-TIME:19991209T100000Z DTEND;VALUE=DATE-TIME:19991209T130000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032417@cern.ch DESCRIPTION:Lecture 3\nAlmost a century after the invention of the proport ional counter\, a large research effort is still devoted to better underst and the basic properties of gaseous detectors\, and to improve their perfo rmances and reliability\, particularly in view of use at the high radiatio n levels expected at LHC. In the first part of the lectures\, after a brie f introduction on underlying physical phenomena\, I will review modern sop histicated computational tools\, as well as some classic 'back \nof the en velope' analytical methods\, available today for estimating the general pe rformances of gaseous detectors. In the second part\, I will analyse in mo re detail problems specific to the use of detectors at high rates (space c harge\, discharges\, aging)\, and describe the recent development of power ful and perhaps more reliable devices\, particularly in the field of posit ion-sensitive micro-pattern detectors.\n\nhttp://indico.cern.ch/conference Display.py?confId=a032417 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032417 END:VEVENT BEGIN:VEVENT SUMMARY:Basic Processes and Trends in Gaseous Detectors\n DTSTART;VALUE=DATE-TIME:19991210T100000Z DTEND;VALUE=DATE-TIME:19991210T130000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032418@cern.ch DESCRIPTION:Lecture 4\nAlmost a century after the invention of the proport ional counter\, a large research effort is still devoted to better underst and the basic properties of gaseous detectors\, and to improve their perfo rmances and reliability\, particularly in view of use at the high radiatio n levels expected at LHC. In the first part of the lectures\, after a brie f introduction on underlying physical phenomena\, I will review modern sop histicated computational tools\, as well as some classic 'back \nof the en velope' analytical methods\, available today for estimating the general pe rformances of gaseous detectors. In the second part\, I will analyse in mo re detail problems specific to the use of \ndetectors at high rates (space charge\, discharges\, aging)\, and describe the recent development of pow erful and perhaps more reliable devices\, particularly in the field of pos ition-sensitive micro-pattern detectors.\n\nhttp://indico.cern.ch/conferen ceDisplay.py?confId=a032418 LOCATION:CERN Council Chamber URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032418 END:VEVENT BEGIN:VEVENT SUMMARY:Telling the truth with statistics\n DTSTART;VALUE=DATE-TIME:20000110T100000Z DTEND;VALUE=DATE-TIME:20000110T153000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032419@cern.ch DESCRIPTION:Lecture 1\n\nHow to tell the truth with Statistics?\nLying wit h statistics is easy.\nA greater challenge is to use statistics to communi cate an accurate and objective summary of given experimental data.\nWe wil l follow both the Bayesian and classical (frequents) approaches to this pr oblem\, and will see that in both cases the key to getting the right answe rs will be to ask meaningful questions.\nA working knowledge of elementary statistics will be assumed\, so that we can concentrate on exact methods and questions of interpretation.\n\nhttp://indico.cern.ch/conferenceDispla y.py?confId=a032419 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032419 END:VEVENT BEGIN:VEVENT SUMMARY:Telling the truth with statistics DTSTART;VALUE=DATE-TIME:20000111T100000Z DTEND;VALUE=DATE-TIME:20000111T101500Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032420@cern.ch DESCRIPTION:Lecture 2\n\nHow to tell the truth with Statistics?\nLying wit h statistics is easy.\nA greater challenge is to use statistics to communi cate an accurate and objective summary of given experimental data.\nWe wil l follow both the Bayesian and classical (frequents) approaches to this pr oblem\, and will see that in both cases the key to getting the right answe rs will be to ask meaningful questions.\nA working knowledge of elementary statistics will be assumed\, so that we can concentrate on exact methods and questions of interpretation.\n\nhttp://indico.cern.ch/conferenceDispla y.py?confId=a032420 LOCATION:CERN Council Chamber URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032420 END:VEVENT BEGIN:VEVENT SUMMARY:Telling the truth with statistics\n DTSTART;VALUE=DATE-TIME:20000112T100000Z DTEND;VALUE=DATE-TIME:20000112T130000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032421@cern.ch DESCRIPTION:Lecture 3\n\nHow to tell the truth with Statistics?\nLying wit h statistics is easy.\nA greater challenge is to use statistics to communi cate an accurate and objective summary of given experimental data.\nWe wil l follow both the Bayesian and classical (frequents) approaches to this pr oblem\, and will see that in both cases the key to getting the right answe rs will be to ask meaningful questions.\n\nA working knowledge of elementa ry statistics will be assumed\, so that we can concentrate on exact method s and questions of interpretation.\n\nhttp://indico.cern.ch/conferenceDisp lay.py?confId=a032421 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032421 END:VEVENT BEGIN:VEVENT SUMMARY:Telling the truth with statistics\n DTSTART;VALUE=DATE-TIME:20000113T100000Z DTEND;VALUE=DATE-TIME:20000113T131500Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032422@cern.ch DESCRIPTION:Lecture 4\n\nHow to tell the truth with Statistics?\nLying wit h statistics is easy.\nA greater challenge is to use statistics to communi cate an accurate and objective summary of given experimental data.\n\nWe w ill follow both the Bayesian and classical (frequents) approaches to this problem\, and will see that in both cases the key to getting the right ans wers will be to ask meaningful questions.\n\nA working knowledge of elemen tary statistics will be assumed\, so that we can concentrate on exact meth ods and questions of interpretation.\n\nhttp://indico.cern.ch/conferenceDi splay.py?confId=a032422 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032422 END:VEVENT BEGIN:VEVENT SUMMARY:Telling the truth with statistics\n DTSTART;VALUE=DATE-TIME:20000114T100000Z DTEND;VALUE=DATE-TIME:20000114T101500Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032423@cern.ch DESCRIPTION:Lecture 5\n\nHow to tell the truth with Statistics?\nLying wit h statistics is easy.\nA greater challenge is to use statistics to communi cate an accurate and objective summary of given experimental data.\n\nWe w ill follow both the Bayesian and classical (frequents) approaches to this problem\, and will see that in both cases the key to getting the right ans wers will be to ask meaningful questions.\n\nA working knowledge of elemen tary statistics will be assumed\, so that we can concentrate on exact meth ods and questions of interpretation.\n\nhttp://indico.cern.ch/conferenceDi splay.py?confId=a032423 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032423 END:VEVENT BEGIN:VEVENT SUMMARY:Advanced materials for application to high energy physics\n DTSTART;VALUE=DATE-TIME:20000117T100000Z DTEND;VALUE=DATE-TIME:20000117T130000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032424@cern.ch DESCRIPTION:Lecture 1\n1a) The crystalline lattice and lattice defects\n1b ) Comments on the materials' cycle\n2a) A general view of the different cl asses of materials\n2b) Thermodynamics as a guide\n3) Reactions between an alloy and its environment (corrosion)\n4) Mechanical strength\, rupture\, the dislocation model\n5a) Techniques of fabrication - old and new ideas\ n5b) Conclusions and outlook\n\nhttp://indico.cern.ch/conferenceDisplay.py ?confId=a032424 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032424 END:VEVENT BEGIN:VEVENT SUMMARY:Advanced materials for application to high energy physics\n DTSTART;VALUE=DATE-TIME:20000118T100000Z DTEND;VALUE=DATE-TIME:20000118T130000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032425@cern.ch DESCRIPTION:Lecture 2\n1a) The crystalline lattice and lattice defects\n1b ) Comments on the materials' cycle\n2a) A general view of the different cl asses of materials\n2b) Thermodynamics as a guide\n3) Reactions between an alloy and its environment (corrosion)\n4) Mechanical strength\, rupture\, the dislocation model\n5a) Techniques of fabrication - old and new ideas\ n5b) Conclusions and outlook\n\nhttp://indico.cern.ch/conferenceDisplay.py ?confId=a032425 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032425 END:VEVENT BEGIN:VEVENT SUMMARY:Advanced materials for application to high energy physics\n DTSTART;VALUE=DATE-TIME:20000119T100000Z DTEND;VALUE=DATE-TIME:20000119T130000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032426@cern.ch DESCRIPTION:Lecture 3\n1a) The crystalline lattice and lattice defects\n1b ) Comments on the materials' cycle\n2a) A general view of the different cl asses of materials\n2b) Thermodynamics as a guide\n3) Reactions between an alloy and its environment (corrosion)\n4) Mechanical strength\, rupture\, the dislocation model\n5a) Techniques of fabrication - old and new ideas\ n5b) Conclusions and outlook\n\nhttp://indico.cern.ch/conferenceDisplay.py ?confId=a032426 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032426 END:VEVENT BEGIN:VEVENT SUMMARY:Advanced materials for application to high energy physics\n DTSTART;VALUE=DATE-TIME:20000120T100000Z DTEND;VALUE=DATE-TIME:20000120T101500Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032427@cern.ch DESCRIPTION:Lecture 4\n1a) The crystalline lattice and lattice defects\n1b ) Comments on the materials' cycle\n2a) A general view of the different cl asses of materials\n2b) Thermodynamics as a guide\n3) Reactions between an alloy and its environment (corrosion)\n4) Mechanical strength\, rupture\, the dislocation model\n5a) Techniques of fabrication - old and new ideas\ n5b) Conclusions and outlook\n\nhttp://indico.cern.ch/conferenceDisplay.py ?confId=a032427 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032427 END:VEVENT BEGIN:VEVENT SUMMARY:Advanced materials for application to high energy physics\n DTSTART;VALUE=DATE-TIME:20000121T100000Z DTEND;VALUE=DATE-TIME:20000121T130000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032428@cern.ch DESCRIPTION:Lecture 5\n1a) The crystalline lattice and lattice defects\n1b ) Comments on the materials' cycle\n2a) A general view of the different cl asses of materials\n2b) Thermodynamics as a guide\n3) Reactions between an alloy and its environment (corrosion)\n4) Mechanical strength\, rupture\, the dislocation model\n5a) Techniques of fabrication - old and new ideas\ n5b) Conclusions and outlook\n\nhttp://indico.cern.ch/conferenceDisplay.py ?confId=a032428 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032428 END:VEVENT BEGIN:VEVENT SUMMARY:Radiation damage in semiconducting devices\, calorimeters and elec tronics\n DTSTART;VALUE=DATE-TIME:20000131T100000Z DTEND;VALUE=DATE-TIME:20000131T130000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032429@cern.ch DESCRIPTION:Lecture 1\nDetector systems at the LHC will have to survive a harsh radiation environment. These lectures will explain the underlying ph ysical basis to radiation effects in various detector systems and associat ed electronics. Four key issues will be discussed: how to relate \nmicrosc opic damage with macroscopic observations\, prediction strategy for a dete ctor system in a known radiation environment with worked examples\, radiat ion testing and monitoring\, outlook for silicon in extreme radiation envi ronments.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a032429 LOCATION:CERN Council Chamber URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032429 END:VEVENT BEGIN:VEVENT SUMMARY:Radiation damage in semiconducting devices\, calorimeters and elec tronics\n DTSTART;VALUE=DATE-TIME:20000201T100000Z DTEND;VALUE=DATE-TIME:20000201T101500Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032430@cern.ch DESCRIPTION:Lecture 2\nDetector systems at the LHC will have to survive a harsh radiation environment. These lectures will explain the underlying ph ysical basis to radiation effects in various detector systems and associat ed electronics. Four key issues will be discussed: how to relate \nmicrosc opic damage with macroscopic observations\, prediction strategy for a dete ctor system in a known radiation environment with worked examples\, radiat ion testing and monitoring\, outlook for silicon in extreme radiation envi ronments.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a032430 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032430 END:VEVENT BEGIN:VEVENT SUMMARY:Radiation damage in semiconducting devices\, calorimeters and elec tronics\n DTSTART;VALUE=DATE-TIME:20000202T100000Z DTEND;VALUE=DATE-TIME:20000202T130000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032431@cern.ch DESCRIPTION:Lecture 3\nDetector systems at the LHC will have to survive a harsh radiation environment. These lectures will explain the underlying ph ysical basis to radiation effects in various detector systems and associat ed electronics. Four key issues will be discussed: how to relate \nmicrosc opic damage with macroscopic observations\, prediction strategy for a dete ctor system in a known radiation environment with worked examples\, radiat ion testing and monitoring\, outlook for silicon in extreme radiation envi ronments.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a032431 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032431 END:VEVENT BEGIN:VEVENT SUMMARY:Radiation damage in semiconducting devices\, calorimeters and elec tronics\n DTSTART;VALUE=DATE-TIME:20000203T100000Z DTEND;VALUE=DATE-TIME:20000203T130000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032432@cern.ch DESCRIPTION:Lecture 4\nDetector systems at the LHC will have to survive a harsh radiation environment. These lectures will explain the underlying ph ysical basis to radiation effects in various detector systems and associat ed electronics. Four key issues will be discussed: how to relate \nmicrosc opic damage with macroscopic observations\, prediction strategy for a dete ctor system in a known radiation environment with worked examples\, radiat ion testing and monitoring\, outlook for silicon in extreme radiation envi ronments.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a032432 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032432 END:VEVENT BEGIN:VEVENT SUMMARY:Radiation damage in semiconducting devices\, calorimeters and elec tronics\n DTSTART;VALUE=DATE-TIME:20000204T100000Z DTEND;VALUE=DATE-TIME:20000204T130000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032433@cern.ch DESCRIPTION:Lecture 5\nDetector systems at the LHC will have to survive a harsh radiation environment. These lectures will explain the underlying ph ysical basis to radiation effects in various detector systems and associat ed electronics. Four key issues will be discussed: how to relate \nmicrosc opic damage with macroscopic observations\, prediction strategy for a dete ctor system in a known radiation environment with worked examples\, radiat ion testing and monitoring\, outlook for silicon in extreme radiation envi ronments.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a032433 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032433 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to particle accelerators\n DTSTART;VALUE=DATE-TIME:20000911T080000Z DTEND;VALUE=DATE-TIME:20000911T081500Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032439@cern.ch DESCRIPTION:This course is recommended as an essential preparation for tho se about to attend the CERN Accelerator School course in October at Loutra ki but is also of interest to a much wider audience - indeed anyone with a technical or scientific background who would like to become familiar with the principles of accelerator design. No specialist knowledge of accelera tor theory is needed but a passing familiarity with Maxwell's equations\, matrix algebra and the solution of second order differential equations wil l be frequently exercised. The series of 10 talks span all aspects of circ ular machines and cover in a simple way the principles of focusing\, betat ron motion\, dispersion\, chromaticity\, radio-frequency systems\, phase s tability and beam instabilities.\n10:00 - Physics of Accelerators \n11:00 - History of Accelerators\n\nhttp://indico.cern.ch/conferenceDisplay.py?co nfId=a032439 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032439 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to particle accelerators\n DTSTART;VALUE=DATE-TIME:20000912T080000Z DTEND;VALUE=DATE-TIME:20000912T120000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032440@cern.ch DESCRIPTION:This course is recommended as an essential preparation for tho se about to attend the CERN Accelerator School course in October at Loutra ki but is also of interest to a much wider audience - indeed anyone with a technical or scientific background who would like to become familiar with the principles of accelerator design. No specialist knowledge of accelera tor theory is needed but a passing familiarity with Maxwell's equations\, matrix algebra and the solution of second order differential equations wil l be frequently exercised. The series of 10 talks span all aspects of circ ular machines and cover in a simple way the principles of focusing\, betat ron motion\, dispersion\, chromaticity\, radio-frequency systems\, phase s tability and beam instabilities.\n10:00 - Principles of Accelerators \n11: 00 - Accelerating Cavities\n\nhttp://indico.cern.ch/conferenceDisplay.py?c onfId=a032440 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032440 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to particle accelerators\n DTSTART;VALUE=DATE-TIME:20000913T080000Z DTEND;VALUE=DATE-TIME:20000913T081500Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032441@cern.ch DESCRIPTION:This course is recommended as an essential preparation for tho se about to attend the CERN Accelerator School course in October at Loutra ki but is also of interest to a much wider audience - indeed anyone with a technical or scientific background who would like to become familiar with the principles of accelerator design. No specialist knowledge of accelera tor theory is needed but a passing familiarity with Maxwell's equations\, matrix algebra and the solution of second order differential equations wil l be frequently exercised. The series of 10 talks span all aspects of circ ular machines and cover in a simple way the principles of focusing\, betat ron motion\, dispersion\, chromaticity\, radio-frequency systems\, phase s tability and beam instabilities.\n10:00 - Lattices \n11:00 - Circulating B eams\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a032441 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032441 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to particle accelerators\n DTSTART;VALUE=DATE-TIME:20000914T080000Z DTEND;VALUE=DATE-TIME:20000914T081500Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032442@cern.ch DESCRIPTION:This course is recommended as an essential preparation for tho se about to attend the CERN Accelerator School course in October at Loutra ki but is also of interest to a much wider audience - indeed anyone with a technical or scientific background who would like to become familiar with the principles of accelerator design. No specialist knowledge of accelera tor theory is needed but a passing familiarity with Maxwell's equations\, matrix algebra and the solution of second order differential equations wil l be frequently exercised. The series of 10 talks span all aspects of circ ular machines and cover in a simple way the principles of focusing\, betat ron motion\, dispersion\, chromaticity\, radio-frequency systems\, phase s tability and beam instabilities.\n10:00 - Longitudinal Dynamics \n11:00 - Imperfections and Multipoles\n\nhttp://indico.cern.ch/conferenceDisplay.py ?confId=a032442 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032442 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to particle accelerators DTSTART;VALUE=DATE-TIME:20000915T080000Z DTEND;VALUE=DATE-TIME:20000915T120000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032443@cern.ch DESCRIPTION:This course is recommended as an essential preparation for tho se about to attend the CERN Accelerator School course in October at Loutra ki but is also of interest to a much wider audience - indeed anyone with a technical or scientific background who would like to become familiar with the principles of accelerator design. No specialist knowledge of accelera tor theory is needed but a passing familiarity with Maxwell's equations\, matrix algebra and the solution of second order differential equations wil l be frequently exercised. The series of 10 talks span all aspects of circ ular machines and cover in a simple way the principles of focusing\, betat ron motion\, dispersion\, chromaticity\, radio-frequency systems\, phase s tability and beam instabilities.\n10:00 - Electrons \n11:00 - Instabilitie s\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a032443 LOCATION:CERN Council Chamber URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032443 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to Field Theory (1/5) DTSTART;VALUE=DATE-TIME:20001023T080000Z DTEND;VALUE=DATE-TIME:20001023T081500Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032444@cern.ch DESCRIPTION:Starting from the notion of path integrals as developed by Fey nman\, we discuss field theory in zero space-time dimensions. The concepts of perturbation expansions\, connected amplitudes\, Feynman diagrams\, cl assical solutions\, renormalization and the effective action are developed . The model is extended to four space-time dimensions\, and the full Feynm an rules for relativistic scalar theory derived. \nThe S matrix and the co ncept of unitarity are discussed\, leading \nto the amputation rules for S matrix elements from considerations of unitarity. The rules are extended to include particles with spin-1/2 and spin-1. The high-energy behaviour o f the theory is discussed as a method to derive the gauge symmetry of the various models.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a0324 44 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032444 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to Field Theory (2/5) DTSTART;VALUE=DATE-TIME:20001024T080000Z DTEND;VALUE=DATE-TIME:20001024T120000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032445@cern.ch DESCRIPTION:Starting from the notion of path integrals as developed by Fey nman\, we discuss field theory in zero space-time dimensions. The concepts of perturbation expansions\, connected amplitudes\, Feynman diagrams\, cl assical solutions\, renormalization and the effective action are developed . The model is extended to four space-time dimensions\, and the full Feynm an rules for relativistic scalar theory derived. \nThe S matrix and the co ncept of unitarity are discussed\, leading \nto the amputation rules for S matrix elements from considerations of unitarity. The rules are extended to include particles with spin-1/2 and spin-1. The high-energy behaviour o f the theory is discussed as a method to derive the gauge symmetry of the various models.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a0324 45 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032445 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to Field Theory (3/5) DTSTART;VALUE=DATE-TIME:20001025T080000Z DTEND;VALUE=DATE-TIME:20001025T120000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032446@cern.ch DESCRIPTION:Starting from the notion of path integrals as developed by Fey nman\, we discuss field theory in zero space-time dimensions. The concepts of perturbation expansions\, connected amplitudes\, Feynman diagrams\, cl assical solutions\, renormalization and the effective action are developed . The model is extended to four space-time dimensions\, and the full Feynm an rules for relativistic scalar theory derived. \nThe S matrix and the co ncept of unitarity are discussed\, leading \nto the amputation rules for S matrix elements from considerations of unitarity. The rules are extended to include particles with spin-1/2 and spin-1. The high-energy behaviour o f the theory is discussed as a method to derive the gauge symmetry of the various models.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a0324 46 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032446 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to Field Theory (4/5) DTSTART;VALUE=DATE-TIME:20001026T080000Z DTEND;VALUE=DATE-TIME:20001026T140000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032447@cern.ch DESCRIPTION:Starting from the notion of path integrals as developed by Fey nman\, we discuss field theory in zero space-time dimensions. The concepts of perturbation expansions\, connected amplitudes\, Feynman diagrams\, cl assical solutions\, renormalization and the effective action are developed . The model is extended to four space-time dimensions\, and the full Feynm an rules for relativistic scalar theory derived. \nThe S matrix and the co ncept of unitarity are discussed\, leading \nto the amputation rules for S matrix elements from considerations of unitarity. The rules are extended to include particles with spin-1/2 and spin-1. The high-energy behaviour o f the theory is discussed as a method to derive the gauge symmetry of the various models.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a0324 47 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032447 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to Field Theory (5/5) DTSTART;VALUE=DATE-TIME:20001027T080000Z DTEND;VALUE=DATE-TIME:20001027T120000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032448@cern.ch DESCRIPTION:Starting from the notion of path integrals as developed by Fey nman\, we discuss field theory in zero space-time dimensions. The concepts of perturbation expansions\, connected amplitudes\, Feynman diagrams\, cl assical solutions\, renormalization and the effective action are developed . The model is extended to four space-time dimensions\, and the full Feynm an rules for relativistic scalar theory derived. \nThe S matrix and the co ncept of unitarity are discussed\, leading \nto the amputation rules for S matrix elements from considerations of unitarity. The rules are extended to include particles with spin-1/2 and spin-1. The high-energy behaviour o f the theory is discussed as a method to derive the gauge symmetry of the various models.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a0324 48 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032448 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to QCD (1) DTSTART;VALUE=DATE-TIME:20001030T090000Z DTEND;VALUE=DATE-TIME:20001030T091500Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032449@cern.ch DESCRIPTION:The course will cover the main features of perturbative QCD\, together with some non-perturbative aspects such as hadronization\, fragme ntation functions and parton distributions in hadrons. Applications to a w ide variety of processes in electron-positron\, lepton-hadron and hadron-h adron collisions will be presented. The theoretical basis of QCD Monte Car lo event generators will also be outlined. Some familiarity with basic qua ntum field theory (Lagrangians\, Dirac algebra\, Feynman graphs) will be a ssumed.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a032449 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032449 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to QCD (2) DTSTART;VALUE=DATE-TIME:20001031T090000Z DTEND;VALUE=DATE-TIME:20001031T091500Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032450@cern.ch DESCRIPTION:The course will cover the main features of perturbative QCD\, together with some non-perturbative aspects such as hadronization\, fragme ntation functions and parton distributions in hadrons. Applications to a w ide variety of processes in electron-positron\, lepton-hadron and hadron-h adron collisions will be presented. The theoretical basis of QCD Monte Car lo event generators will also be outlined. Some familiarity with basic qua ntum field theory (Lagrangians\, Dirac algebra\, Feynman graphs) will be a ssumed.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a032450 LOCATION:CERN Council Chamber URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032450 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to QCD (3) DTSTART;VALUE=DATE-TIME:20001101T090000Z DTEND;VALUE=DATE-TIME:20001101T143000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032451@cern.ch DESCRIPTION:The course will cover the main features of perturbative QCD\, together with some non-perturbative aspects such as hadronization\, fragme ntation functions and parton distributions in hadrons. Applications to a w ide variety of processes in electron-positron\, lepton-hadron and hadron-h adron collisions will be presented. The theoretical basis of QCD Monte Car lo event generators will also be outlined. Some familiarity with basic qua ntum field theory (Lagrangians\, Dirac algebra\, Feynman graphs) will be a ssumed.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a032451 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032451 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to QCD (4) DTSTART;VALUE=DATE-TIME:20001102T090000Z DTEND;VALUE=DATE-TIME:20001102T091500Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032452@cern.ch DESCRIPTION:The course will cover the main features of perturbative QCD\, together with some non-perturbative aspects such as hadronization\, fragme ntation functions and parton distributions in hadrons. Applications to a w ide variety of processes in electron-positron\, lepton-hadron and hadron-h adron collisions will be presented. The theoretical basis of QCD Monte Car lo event generators will also be outlined. Some familiarity with basic qua ntum field theory (Lagrangians\, Dirac algebra\, Feynman graphs) will be a ssumed.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a032452 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032452 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to QCD (5) / Please note that time has changed DTSTART;VALUE=DATE-TIME:20001103T100000Z DTEND;VALUE=DATE-TIME:20001103T225900Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032453@cern.ch DESCRIPTION:The course will cover the main features of perturbative QCD\, together with some non-perturbative aspects such as hadronization\, fragme ntation functions and parton distributions in hadrons. Applications to a w ide variety of processes in electron-positron\, lepton-hadron and hadron-h adron collisions will be presented. The theoretical basis of QCD Monte Car lo event generators will also be outlined. Some familiarity with basic qua ntum field theory (Lagrangians\, Dirac algebra\, Feynman graphs) will be a ssumed.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a032453 LOCATION:CERN Council Chamber URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032453 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to the Standard Model (1/5) DTSTART;VALUE=DATE-TIME:20001120T090000Z DTEND;VALUE=DATE-TIME:20001120T100000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032454@cern.ch DESCRIPTION:The construction of the standard gauge theory of weak and elec tromagnetic interactions (the Standard Model) will be described in detail\ , starting from phenomenological evidences and theoretical prejudices. Spe cial attention will be devoted to the internal consistency of the theory ( gauge invariance and anomaly cancellation). The mechanism of generation of particle masses\, and the violation of flavour symmetries will be illustr ated.\n\nIn the second part of the lectures\, some more specific topics\, such as theoretical bounds on the Higgs boson mass\, and the violation of the CP invariance in the standard model\, will be discussed.\n\nhttp://ind ico.cern.ch/conferenceDisplay.py?confId=a032454 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032454 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to the Standard Model (2/5) DTSTART;VALUE=DATE-TIME:20001121T090000Z DTEND;VALUE=DATE-TIME:20001121T100000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032455@cern.ch DESCRIPTION:The construction of the standard gauge theory of weak and elec tromagnetic interactions (the Standard Model) will be described in detail\ , starting from phenomenological evidences and theoretical prejudices. Spe cial attention will be devoted to the internal consistency of the theory ( gauge invariance and anomaly cancellation). The mechanism of generation of particle masses\, and the violation of flavour symmetries will be illustr ated.\n\nIn the second part of the lectures\, some more specific topics\, such as theoretical bounds on the Higgs boson mass\, and the violation of the CP invariance in the standard model\, will be discussed.\n\nhttp://ind ico.cern.ch/conferenceDisplay.py?confId=a032455 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032455 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to the Standard Model (3/5) DTSTART;VALUE=DATE-TIME:20001122T090000Z DTEND;VALUE=DATE-TIME:20001122T100000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032456@cern.ch DESCRIPTION:The construction of the standard gauge theory of weak and elec tromagnetic interactions (the Standard Model) will be described in detail\ , starting from phenomenological evidences and theoretical prejudices. Spe cial attention will be devoted to the internal consistency of the theory ( gauge invariance and anomaly cancellation). The mechanism of generation of particle masses\, and the violation of flavour symmetries will be illustr ated.\n\nIn the second part of the lectures\, some more specific topics\, such as theoretical bounds on the Higgs boson mass\, and the violation of the CP invariance in the standard model\, will be discussed.\n\nhttp://ind ico.cern.ch/conferenceDisplay.py?confId=a032456 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032456 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to the Standard Model (4/5) DTSTART;VALUE=DATE-TIME:20001123T090000Z DTEND;VALUE=DATE-TIME:20001123T100000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032457@cern.ch DESCRIPTION:The construction of the standard gauge theory of weak and elec tromagnetic interactions (the Standard Model) will be described in detail\ , starting from phenomenological evidences and theoretical prejudices. Spe cial attention will be devoted to the internal consistency of the theory ( gauge invariance and anomaly cancellation). The mechanism of generation of particle masses\, and the violation of flavour symmetries will be illustr ated.\n\nIn the second part of the lectures\, some more specific topics\, such as theoretical bounds on the Higgs boson mass\, and the violation of the CP invariance in the standard model\, will be discussed.\n\nhttp://ind ico.cern.ch/conferenceDisplay.py?confId=a032457 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032457 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to the Standard Model (5/5) DTSTART;VALUE=DATE-TIME:20001124T090000Z DTEND;VALUE=DATE-TIME:20001124T100000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032458@cern.ch DESCRIPTION:The construction of the standard gauge theory of weak and elec tromagnetic interactions (the Standard Model) will be described in detail\ , starting from phenomenological evidences and theoretical prejudices. Spe cial attention will be devoted to the internal consistency of the theory ( gauge invariance and anomaly cancellation). The mechanism of generation of particle masses\, and the violation of flavour symmetries will be illustr ated.\n\nIn the second part of the lectures\, some more specific topics\, such as theoretical bounds on the Higgs boson mass\, and the violation of the CP invariance in the standard model\, will be discussed.\n\nhttp://ind ico.cern.ch/conferenceDisplay.py?confId=a032458 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032458 END:VEVENT BEGIN:VEVENT SUMMARY:Beyond the Standard Model (1/5) DTSTART;VALUE=DATE-TIME:20001211T100000Z DTEND;VALUE=DATE-TIME:20001211T220000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032434@cern.ch DESCRIPTION:After a critical discussion of the questions left unanswered b y the \nStandard Model\, I will review the main attemps to construct new t heories. In particular\, I will discuss grand unification\, supersymmetry\ , technicolour\, and theories with extra dimensions.\n\nhttp://indico.cern .ch/conferenceDisplay.py?confId=a032434 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032434 END:VEVENT BEGIN:VEVENT SUMMARY:Beyond the Standard Model (2/5) DTSTART;VALUE=DATE-TIME:20001212T100000Z DTEND;VALUE=DATE-TIME:20001212T220000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032435@cern.ch DESCRIPTION:After a critical discussion of the questions left unanswered b y the \nStandard Model\, I will review the main attemps to construct new t heories. In particular\, I will discuss grand unification\, supersymmetry\ , technicolour\, and theories with extra dimensions.\n\nhttp://indico.cern .ch/conferenceDisplay.py?confId=a032435 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032435 END:VEVENT BEGIN:VEVENT SUMMARY:Beyond the Standard Model (3/5) DTSTART;VALUE=DATE-TIME:20001213T100000Z DTEND;VALUE=DATE-TIME:20001213T220000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032436@cern.ch DESCRIPTION:After a critical discussion of the questions left unanswered b y the \nStandard Model\, I will review the main attemps to construct new t heories. In particular\, I will discuss grand unification\, supersymmetry\ , technicolour\, and theories with extra dimensions.\n\nhttp://indico.cern .ch/conferenceDisplay.py?confId=a032436 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032436 END:VEVENT BEGIN:VEVENT SUMMARY:Beyond the Standard Model (4/5) DTSTART;VALUE=DATE-TIME:20001214T100000Z DTEND;VALUE=DATE-TIME:20001214T220000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032437@cern.ch DESCRIPTION:After a critical discussion of the questions left unanswered b y the \nStandard Model\, I will review the main attemps to construct new t heories. In particular\, I will discuss grand unification\, supersymmetry\ , technicolour\, and theories with extra dimensions.\n\nhttp://indico.cern .ch/conferenceDisplay.py?confId=a032437 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032437 END:VEVENT BEGIN:VEVENT SUMMARY:Beyond the Standard Model (5/5) DTSTART;VALUE=DATE-TIME:20001215T100000Z DTEND;VALUE=DATE-TIME:20001215T220000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032438@cern.ch DESCRIPTION:After a critical discussion of the questions left unanswered b y the \nStandard Model\, I will review the main attemps to construct new t heories. In particular\, I will discuss grand unification\, supersymmetry\ , technicolour\, and theories with extra dimensions.\n\nhttp://indico.cern .ch/conferenceDisplay.py?confId=a032438 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032438 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to particle accelerators - 10 talks DTSTART;VALUE=DATE-TIME:20011001T080000Z DTEND;VALUE=DATE-TIME:20011001T080000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032464@cern.ch DESCRIPTION:This new series of lectures is intended for anyone with a tech nical or scientific background who would like to become familiar with the principles of accelerator design. It is a complement to last year's course and includes new lectures on present day accelerators\, and their applica tions as well as colliders and neutrino factories. Beam dynamics\, which w as treated at length in last year's course\, has been compressed into one lecture\, intended as revision for those who followed earlier courses and an introduction for newcomers to the field. The course should not be misse d by those who will attend the CAS Intermediate Accelerator School in Sevi lle.\n\nThe reference work for the Course is 'An Introduction to Particle Accelerators'\nhttp://www.oup.co.uk/isbn/0-19-850829-8\n\nThose who wish t o prepare themselves thoroughly for Beam Dynamics may find it useful to vi ew four of last year's web archived lectures:\n\nhttp://webcast.cern.ch/Pr ojects/WebLectureArchive/acad/2000/wilson/3/f001.htm\n\nhttp://webcast.cer n.ch/Projects/WebLectureArchive/acad/2000/wilson/5/f001.htm\n\nhttp://webc ast.cern.ch/Projects/WebLectureArchive/acad/2000/wilson/6/f001.htm\n\nhttp ://webcast.cern.ch/Projects/WebLectureArchive/acad/2000/wilson/7/f001.htm\ n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a032464 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032464 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to particle accelerators (1/10) DTSTART;VALUE=DATE-TIME:20011001T080000Z DTEND;VALUE=DATE-TIME:20011001T090000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032465@cern.ch DESCRIPTION:Present-day Accelerators\n\nhttp://indico.cern.ch/conferenceDi splay.py?confId=a032465 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032465 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to particle accelerators (2/10) DTSTART;VALUE=DATE-TIME:20011001T090000Z DTEND;VALUE=DATE-TIME:20011001T100000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032474@cern.ch DESCRIPTION:Beam Dynamics\n\nhttp://indico.cern.ch/conferenceDisplay.py?co nfId=a032474 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032474 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to particle accelerators (3/10) DTSTART;VALUE=DATE-TIME:20011002T080000Z DTEND;VALUE=DATE-TIME:20011002T090000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032466@cern.ch DESCRIPTION:Accelerating Cavities\n\nhttp://indico.cern.ch/conferenceDispl ay.py?confId=a032466 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032466 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to particle accelerators (4/10) DTSTART;VALUE=DATE-TIME:20011002T090000Z DTEND;VALUE=DATE-TIME:20011002T100000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032467@cern.ch DESCRIPTION:Non-linear Dynamics\n\nhttp://indico.cern.ch/conferenceDisplay .py?confId=a032467 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032467 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to particle accelerators (5/10) DTSTART;VALUE=DATE-TIME:20011003T080000Z DTEND;VALUE=DATE-TIME:20011003T090000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032468@cern.ch DESCRIPTION:Electron Dynamics\n\nhttp://indico.cern.ch/conferenceDisplay.p y?confId=a032468 LOCATION:CERN Council Chamber URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032468 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to particle accelerators (6/10) DTSTART;VALUE=DATE-TIME:20011003T090000Z DTEND;VALUE=DATE-TIME:20011003T100000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032473@cern.ch DESCRIPTION:Instabilities\n\nhttp://indico.cern.ch/conferenceDisplay.py?co nfId=a032473 LOCATION:CERN Council Chamber URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032473 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to particle accelerators (7/10) DTSTART;VALUE=DATE-TIME:20011004T080000Z DTEND;VALUE=DATE-TIME:20011004T090000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032469@cern.ch DESCRIPTION:Colliders\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId =a032469 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032469 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to particle accelerators (8/10) DTSTART;VALUE=DATE-TIME:20011004T090000Z DTEND;VALUE=DATE-TIME:20011004T100000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032470@cern.ch DESCRIPTION:Neutrino Factory\n\nhttp://indico.cern.ch/conferenceDisplay.py ?confId=a032470 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032470 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to particle accelerators (9/10) DTSTART;VALUE=DATE-TIME:20011005T080000Z DTEND;VALUE=DATE-TIME:20011005T090000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032471@cern.ch DESCRIPTION:Applications of Accelerators\n\nhttp://indico.cern.ch/conferen ceDisplay.py?confId=a032471 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032471 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to particle accelerators (10/10) DTSTART;VALUE=DATE-TIME:20011005T090000Z DTEND;VALUE=DATE-TIME:20011005T100000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032472@cern.ch DESCRIPTION:The Future\n\nhttp://indico.cern.ch/conferenceDisplay.py?confI d=a032472 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032472 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to Field Theory (1/5) DTSTART;VALUE=DATE-TIME:20011008T080000Z DTEND;VALUE=DATE-TIME:20011008T100000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032459@cern.ch DESCRIPTION:Starting from the notion of path integrals as developed by Fey nman\, we discuss field theory in zero spacetime dimensions. The concepts of perturbation expansions\, connected amplitudes\, Feynman diagrams\, cla ssical solutions\, renormalization and the effective action are \ndevelope d. The model is extended to four spacetime dimensions\, and the full Feynm an rules for relativisitc scalar theory derived. \nThe S matrix and the co ncept of unitarity are discussed\, leading to the amputation rules for S m atrix elements from considerations of unitarity. The rules are extended to include particles with spin-1/2 and spin-1. The high-energy behaviour of the theory is discussed as a method to derive the gauge symmetry of the va rious models.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a032459 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032459 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to Field Theory (2/5) DTSTART;VALUE=DATE-TIME:20011009T080000Z DTEND;VALUE=DATE-TIME:20011009T100000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032460@cern.ch DESCRIPTION:Starting from the notion of path integrals as developed by Fey nman\, we discuss field theory in zero spacetime dimensions. The concepts of perturbation expansions\, connected amplitudes\, Feynman diagrams\, cla ssical solutions\, renormalization and the effective action are \ndevelope d. The model is extended to four spacetime dimensions\, and the full Feynm an rules for relativisitc scalar theory derived. \nThe S matrix and the co ncept of unitarity are discussed\, leading to the amputation rules for S m atrix elements from considerations of unitarity. The rules are extended to include particles with spin-1/2 and spin-1. The high-energy behaviour of the theory is discussed as a method to derive the gauge symmetry of the va rious models.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a032460 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032460 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to Field Theory (3/5) DTSTART;VALUE=DATE-TIME:20011010T080000Z DTEND;VALUE=DATE-TIME:20011010T100000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032461@cern.ch DESCRIPTION:Starting from the notion of path integrals as developed by Fey nman\, we discuss field theory in zero spacetime dimensions. The concepts of perturbation expansions\, connected amplitudes\, Feynman diagrams\, cla ssical solutions\, renormalization and the effective action are \ndevelope d. The model is extended to four spacetime dimensions\, and the full Feynm an rules for relativisitc scalar theory derived. \nThe S matrix and the co ncept of unitarity are discussed\, leading to the amputation rules for S m atrix elements from considerations of unitarity. The rules are extended to include particles with spin-1/2 and spin-1. The high-energy behaviour of the theory is discussed as a method to derive the gauge symmetry of the va rious models.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a032461 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032461 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to Field Theory (4/5) DTSTART;VALUE=DATE-TIME:20011011T080000Z DTEND;VALUE=DATE-TIME:20011011T100000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032462@cern.ch DESCRIPTION:Starting from the notion of path integrals as developed by Fey nman\, we discuss field theory in zero spacetime dimensions. The concepts of perturbation expansions\, connected amplitudes\, Feynman diagrams\, cla ssical solutions\, renormalization and the effective action are \ndevelope d. The model is extended to four spacetime dimensions\, and the full Feynm an rules for relativisitc scalar theory derived. \nThe S matrix and the co ncept of unitarity are discussed\, leading to the amputation rules for S m atrix elements from considerations of unitarity. The rules are extended to include particles with spin-1/2 and spin-1. The high-energy behaviour of the theory is discussed as a method to derive the gauge symmetry of the va rious models.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a032462 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032462 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to Field Theory (5/5) DTSTART;VALUE=DATE-TIME:20011012T080000Z DTEND;VALUE=DATE-TIME:20011012T100000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032463@cern.ch DESCRIPTION:Starting from the notion of path integrals as developed by Fey nman\, we discuss field theory in zero spacetime dimensions. The concepts of perturbation expansions\, connected amplitudes\, Feynman diagrams\, cla ssical solutions\, renormalization and the effective action are \ndevelope d. The model is extended to four spacetime dimensions\, and the full Feynm an rules for relativisitc scalar theory derived. \nThe S matrix and the co ncept of unitarity are discussed\, leading to the amputation rules for S m atrix elements from considerations of unitarity. The rules are extended to include particles with spin-1/2 and spin-1. The high-energy behaviour of the theory is discussed as a method to derive the gauge symmetry of the va rious models.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a032463 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032463 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to symmetry breaking phenomena in physics (1/3) DTSTART;VALUE=DATE-TIME:20011121T100000Z DTEND;VALUE=DATE-TIME:20011121T110000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032475@cern.ch DESCRIPTION:The notion of broken symmetries started slowly to emerge in th e 19th century. The early studies of Pasteur on the parity asymmetry of li fe\, the studies of Curie on piezoelectricity and on the symmetries of eff ects versus the symmetry of causes ( which clearly excluded spontaneous sy mmetry breaking)\, are important historical landmarks. However the possibi lity of spontaneous symmetry breaking within the usual principles of stati stical mechanics\, waited for the work of Peierls and Onsager. The whole t heory of phase transitions and critical phenomena\, as well as the constru ction of field theoretic models as long distance limit of yet unknown phys ics\, relies nowadays on the concept of criticality associated to spontane ous symmetry breaking. The phenomena of Goldstone bosons\, of Meissner-Hig gs effects\, are central to the theory of condensed matter as well as to p article physics. In cosmology as well\, the various inflationary scenarios begin similarly with this same concept. The three lectures will provide a simple survey of the notion of symmetry breaking in those various fields. \n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a032475 LOCATION:CERN Council Chamber URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032475 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to symmetry breaking phenomena in physics (2/3) DTSTART;VALUE=DATE-TIME:20011122T100000Z DTEND;VALUE=DATE-TIME:20011122T110000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032476@cern.ch DESCRIPTION:The notion of broken symmetries started slowly to emerge in th e 19th century. The early studies of Pasteur on the parity asymmetry of li fe\, the studies of Curie on piezoelectricity and on the symmetries of eff ects versus the symmetry of causes ( which clearly excluded spontaneous sy mmetry breaking)\, are important historical landmarks. However the possibi lity of spontaneous symmetry breaking within the usual principles of stati stical mechanics\, waited for the work of Peierls and Onsager. The whole t heory of phase transitions and critical phenomena\, as well as the constru ction of field theoretic models as long distance limit of yet unknown phys ics\, relies nowadays on the concept of criticality associated to spontane ous symmetry breaking. The phenomena of Goldstone bosons\, of Meissner-Hig gs effects\, are central to the theory of condensed matter as well as to p article physics. In cosmology as well\, the various inflationary scenarios begin similarly with this same concept. The three lectures will provide a simple survey of the notion of symmetry breaking in those various fields. \n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a032476 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032476 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to symmetry breaking phenomena in physics (3/3) DTSTART;VALUE=DATE-TIME:20011123T100000Z DTEND;VALUE=DATE-TIME:20011123T110000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032477@cern.ch DESCRIPTION:The notion of broken symmetries started slowly to emerge in th e 19th century. The early studies of Pasteur on the parity asymmetry of li fe\, the studies of Curie on piezoelectricity and on the symmetries of eff ects versus the symmetry of causes ( which clearly excluded spontaneous sy mmetry breaking)\, are important historical landmarks. However the possibi lity of spontaneous symmetry breaking within the usual principles of stati stical mechanics\, waited for the work of Peierls and Onsager. The whole t heory of phase transitions and critical phenomena\, as well as the constru ction of field theoretic models as long distance limit of yet unknown phys ics\, relies nowadays on the concept of criticality associated to spontane ous symmetry breaking. The phenomena of Goldstone bosons\, of Meissner-Hig gs effects\, are central to the theory of condensed matter as well as to p article physics. In cosmology as well\, the various inflationary scenarios begin similarly with this same concept. The three lectures will provide a simple survey of the notion of symmetry breaking in those various fields. \n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a032477 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032477 END:VEVENT BEGIN:VEVENT SUMMARY:Telling the Truth with Statistics (1/5) DTSTART;VALUE=DATE-TIME:20021118T100000Z DTEND;VALUE=DATE-TIME:20021118T110000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032478@cern.ch DESCRIPTION:This course of lectures will cover probability\, distributions \, fitting\, errors and confidence levels\, for practising High Energy Phy sicists who need to use Statistical techniques to express their results. C oncentrating on these appropriate specialist techniques means that they ca n be covered in appropriate depth\, while assuming only the knowledge and experience of a typical Particle Physicist.\n\nThe different definitions o f probability will be explained\, and it will be appear why this basic sub ject is so controversial\; there are several viewpoints and it is importan t to understand them all\, rather than abusing the adherents of different beliefs.\n\nDistributions will be covered: the situations they arise in\, their useful properties\, and the amazing result of the Central Limit Theo rem.\n\nFitting a parametrisation to a set of data is one of the most wide spread uses of statistics: these are lots of ways of doing this and these will be presented\, with discussion of which is appropriate in different c ircumstances.\n\nThis then leads to the subject of errors and how to calcu late them\, in which there is a lot of timid overestimation in general pra ctice\, and the whole business of confidence intervals\, where recent expe rimental results (with the signal small or zero) have driven new theoretic al ideas.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a032478 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032478 END:VEVENT BEGIN:VEVENT SUMMARY:Telling the Truth with Statistics (2/5) DTSTART;VALUE=DATE-TIME:20021119T100000Z DTEND;VALUE=DATE-TIME:20021119T110000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032479@cern.ch DESCRIPTION:This course of lectures will cover probability\, distributions \, fitting\, errors and confidence levels\, for practising High Energy Phy sicists who need to use Statistical techniques to express their results. C oncentrating on these appropriate specialist techniques means that they ca n be covered in appropriate depth\, while assuming only the knowledge and experience of a typical Particle Physicist.\n\nThe different definitions o f probability will be explained\, and it will be appear why this basic sub ject is so controversial\; there are several viewpoints and it is importan t to understand them all\, rather than abusing the adherents of different beliefs.\n\nDistributions will be covered: the situations they arise in\, their useful properties\, and the amazing result of the Central Limit Theo rem.\n\nFitting a parametrisation to a set of data is one of the most wide spread uses of statistics: these are lots of ways of doing this and these will be presented\, with discussion of which is appropriate in different c ircumstances.\n\nThis then leads to the subject of errors and how to calcu late them\, in which there is a lot of timid overestimation in general pra ctice\, and the whole business of confidence intervals\, where recent expe rimental results (with the signal small or zero) have driven new theoretic al ideas.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a032479 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032479 END:VEVENT BEGIN:VEVENT SUMMARY:Telling the Truth with Statistics (3/5) DTSTART;VALUE=DATE-TIME:20021120T100000Z DTEND;VALUE=DATE-TIME:20021120T110000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032480@cern.ch DESCRIPTION:This course of lectures will cover probability\, distributions \, fitting\, errors and confidence levels\, for practising High Energy Phy sicists who need to use Statistical techniques to express their results. C oncentrating on these appropriate specialist techniques means that they ca n be covered in appropriate depth\, while assuming only the knowledge and experience of a typical Particle Physicist.\n\nThe different definitions o f probability will be explained\, and it will be appear why this basic sub ject is so controversial\; there are several viewpoints and it is importan t to understand them all\, rather than abusing the adherents of different beliefs.\n\nDistributions will be covered: the situations they arise in\, their useful properties\, and the amazing result of the Central Limit Theo rem.\n\nFitting a parametrisation to a set of data is one of the most wide spread uses of statistics: these are lots of ways of doing this and these will be presented\, with discussion of which is appropriate in different c ircumstances.\n\nThis then leads to the subject of errors and how to calcu late them\, in which there is a lot of timid overestimation in general pra ctice\, and the whole business of confidence intervals\, where recent expe rimental results (with the signal small or zero) have driven new theoretic al ideas.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a032480 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032480 END:VEVENT BEGIN:VEVENT SUMMARY:Telling the Truth with Statistics (4/5) DTSTART;VALUE=DATE-TIME:20021121T100000Z DTEND;VALUE=DATE-TIME:20021121T110000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032481@cern.ch DESCRIPTION:This course of lectures will cover probability\, distributions \, fitting\, errors and confidence levels\, for practising High Energy Phy sicists who need to use Statistical techniques to express their results. C oncentrating on these appropriate specialist techniques means that they ca n be covered in appropriate depth\, while assuming only the knowledge and experience of a typical Particle Physicist.\n\nThe different definitions o f probability will be explained\, and it will be appear why this basic sub ject is so controversial\; there are several viewpoints and it is importan t to understand them all\, rather than abusing the adherents of different beliefs.\n\nDistributions will be covered: the situations they arise in\, their useful properties\, and the amazing result of the Central Limit Theo rem.\n\nFitting a parametrisation to a set of data is one of the most wide spread uses of statistics: these are lots of ways of doing this and these will be presented\, with discussion of which is appropriate in different c ircumstances.\n\nThis then leads to the subject of errors and how to calcu late them\, in which there is a lot of timid overestimation in general pra ctice\, and the whole business of confidence intervals\, where recent expe rimental results (with the signal small or zero) have driven new theoretic al ideas.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a032481 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032481 END:VEVENT BEGIN:VEVENT SUMMARY:Telling the Truth with Statistics (5/5) DTSTART;VALUE=DATE-TIME:20021122T100000Z DTEND;VALUE=DATE-TIME:20021122T110000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032482@cern.ch DESCRIPTION:This course of lectures will cover probability\, distributions \, fitting\, errors and confidence levels\, for practising High Energy Phy sicists who need to use Statistical techniques to express their results. C oncentrating on these appropriate specialist techniques means that they ca n be covered in appropriate depth\, while assuming only the knowledge and experience of a typical Particle Physicist.\n\nThe different definitions o f probability will be explained\, and it will be appear why this basic sub ject is so controversial\; there are several viewpoints and it is importan t to understand them all\, rather than abusing the adherents of different beliefs.\n\nDistributions will be covered: the situations they arise in\, their useful properties\, and the amazing result of the Central Limit Theo rem.\n\nFitting a parametrisation to a set of data is one of the most wide spread uses of statistics: these are lots of ways of doing this and these will be presented\, with discussion of which is appropriate in different c ircumstances.\n\nThis then leads to the subject of errors and how to calcu late them\, in which there is a lot of timid overestimation in general pra ctice\, and the whole business of confidence intervals\, where recent expe rimental results (with the signal small or zero) have driven new theoretic al ideas.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a032482 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032482 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to String Theory (1/4) DTSTART;VALUE=DATE-TIME:20021202T100000Z DTEND;VALUE=DATE-TIME:20021202T110000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032483@cern.ch DESCRIPTION:I will present a simple and non-technical overview of string t heory\, aimed for non-experts who like to get some idea what string theory is about. Besides introductory material\, I intend to cover also some of the more recent developments.\n\nhttp://indico.cern.ch/conferenceDisplay.p y?confId=a032483 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032483 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to String Theory (2/4) DTSTART;VALUE=DATE-TIME:20021203T100000Z DTEND;VALUE=DATE-TIME:20021203T110000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032484@cern.ch DESCRIPTION:I will present a simple and non-technical overview of string t heory\, aimed for non-experts who like to get some idea what string theory is about. Besides introductory material\, I intend to cover also some of the more recent developments.\n\nhttp://indico.cern.ch/conferenceDisplay.p y?confId=a032484 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032484 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to String Theory (3/4) DTSTART;VALUE=DATE-TIME:20021204T100000Z DTEND;VALUE=DATE-TIME:20021204T110000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032485@cern.ch DESCRIPTION:I will present a simple and non-technical overview of string t heory\, aimed for non-experts who like to get some idea what string theory is about. Besides introductory material\, I intend to cover also some of the more recent developments.\n\nhttp://indico.cern.ch/conferenceDisplay.p y?confId=a032485 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032485 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to String Theory (4/4) DTSTART;VALUE=DATE-TIME:20021205T100000Z DTEND;VALUE=DATE-TIME:20021205T110000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a032486@cern.ch DESCRIPTION:I will present a simple and non-technical overview of string t heory\, aimed for non-experts who like to get some idea what string theory is about. Besides introductory material\, I intend to cover also some of the more recent developments.\n\nhttp://indico.cern.ch/conferenceDisplay.p y?confId=a032486 LOCATION:CERN Council Chamber URL:http://indico.cern.ch/conferenceDisplay.py?confId=a032486 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to QCD (1/5)\n DTSTART;VALUE=DATE-TIME:20031020T090000Z DTEND;VALUE=DATE-TIME:20031020T100000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a035234@cern.ch DESCRIPTION:The emphasis of the lectures will be on QCD phenomenology at h igh energy. The main topics of the five lectures will be :\n1) Basics of Q CD: Feynman rules\, running coupling\, beta function\, renormalization sch emes\, infra-red singularities\, non-perturbative QCD.\n2) e+e- & parton b ranching: e+e- total cross section\, shape distributions\, jet fractions\, parton branching\, splitting functions\, jet angular distributions.\n3) E volution equations: DGLAP equation\, Sudakov form factor\, Monte Carlo met hod\, soft gluon emission\, angular ordering\, coherent branching.\n4) Jet fragmentation: Fragmentation functions\, small-x fragmentation\, average multiplicity\, hadronization models\, cluster and string models\, particl e yields and spectra\, quark and gluon jets.\n5) DIS & hadron-hadron proce sses: Deep inelastic scattering\, scaling violation\, small x\, hadron-had ron processes\, lepton pair production\, jet production\, heavy quark prod uction.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a035234 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a035234 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to QCD (2/5)\n DTSTART;VALUE=DATE-TIME:20031021T090000Z DTEND;VALUE=DATE-TIME:20031021T100000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a035235@cern.ch DESCRIPTION:The emphasis of the lectures will be on QCD phenomenology at h igh energy. The main topics of the five lectures will be :\n1) Basics of Q CD: Feynman rules\, running coupling\, beta function\, renormalization sch emes\, infra-red singularities\, non-perturbative QCD.\n2) e+e- & parton b ranching: e+e- total cross section\, shape distributions\, jet fractions\, parton branching\, splitting functions\, jet angular distributions.\n3) E volution equations: DGLAP equation\, Sudakov form factor\, Monte Carlo met hod\, soft gluon emission\, angular ordering\, coherent branching.\n4) Jet fragmentation: Fragmentation functions\, small-x fragmentation\, average multiplicity\, hadronization models\, cluster and string models\, particl e yields and spectra\, quark and gluon jets.\n5) DIS & hadron-hadron proce sses: Deep inelastic scattering\, scaling violation\, small x\, hadron-had ron processes\, lepton pair production\, jet production\, heavy quark prod uction.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a035235 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a035235 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to QCD (3/5)\n DTSTART;VALUE=DATE-TIME:20031022T090000Z DTEND;VALUE=DATE-TIME:20031022T100000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a035236@cern.ch DESCRIPTION:The emphasis of the lectures will be on QCD phenomenology at h igh energy. The main topics of the five lectures will be :\n1) Basics of Q CD: Feynman rules\, running coupling\, beta function\, renormalization sch emes\, infra-red singularities\, non-perturbative QCD.\n2) e+e- & parton b ranching: e+e- total cross section\, shape distributions\, jet fractions\, parton branching\, splitting functions\, jet angular distributions.\n3) E volution equations: DGLAP equation\, Sudakov form factor\, Monte Carlo met hod\, soft gluon emission\, angular ordering\, coherent branching.\n4) Jet fragmentation: Fragmentation functions\, small-x fragmentation\, average multiplicity\, hadronization models\, cluster and string models\, particl e yields and spectra\, quark and gluon jets.\n5) DIS & hadron-hadron proce sses: Deep inelastic scattering\, scaling violation\, small x\, hadron-had ron processes\, lepton pair production\, jet production\, heavy quark prod uction.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a035236 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a035236 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to QCD (4/5)\n DTSTART;VALUE=DATE-TIME:20031023T090000Z DTEND;VALUE=DATE-TIME:20031023T100000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a035237@cern.ch DESCRIPTION:The emphasis of the lectures will be on QCD phenomenology at h igh energy. The main topics of the five lectures will be :\n1) Basics of Q CD: Feynman rules\, running coupling\, beta function\, renormalization sch emes\, infra-red singularities\, non-perturbative QCD.\n2) e+e- & parton b ranching: e+e- total cross section\, shape distributions\, jet fractions\, parton branching\, splitting functions\, jet angular distributions.\n3) E volution equations: DGLAP equation\, Sudakov form factor\, Monte Carlo met hod\, soft gluon emission\, angular ordering\, coherent branching.\n4) Jet fragmentation: Fragmentation functions\, small-x fragmentation\, average multiplicity\, hadronization models\, cluster and string models\, particl e yields and spectra\, quark and gluon jets.\n5) DIS & hadron-hadron proce sses: Deep inelastic scattering\, scaling violation\, small x\, hadron-had ron processes\, lepton pair production\, jet production\, heavy quark prod uction.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a035237 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a035237 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to QCD (5/5)\n DTSTART;VALUE=DATE-TIME:20031024T090000Z DTEND;VALUE=DATE-TIME:20031024T100000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a035238@cern.ch DESCRIPTION:The emphasis of the lectures will be on QCD phenomenology at h igh energy. The main topics of the five lectures will be :\n1) Basics of Q CD: Feynman rules\, running coupling\, beta function\, renormalization sch emes\, infra-red singularities\, non-perturbative QCD.\n2) e+e- & parton b ranching: e+e- total cross section\, shape distributions\, jet fractions\, parton branching\, splitting functions\, jet angular distributions.\n3) E volution equations: DGLAP equation\, Sudakov form factor\, Monte Carlo met hod\, soft gluon emission\, angular ordering\, coherent branching.\n4) Jet fragmentation: Fragmentation functions\, small-x fragmentation\, average multiplicity\, hadronization models\, cluster and string models\, particl e yields and spectra\, quark and gluon jets.\n5) DIS & hadron-hadron proce sses: Deep inelastic scattering\, scaling violation\, small x\, hadron-had ron processes\, lepton pair production\, jet production\, heavy quark prod uction.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a035238 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a035238 END:VEVENT BEGIN:VEVENT SUMMARY:Physics beyond the Standard Model (1/5) DTSTART;VALUE=DATE-TIME:20040329T090000Z DTEND;VALUE=DATE-TIME:20040329T100000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a036621@cern.ch DESCRIPTION:I discuss several issues beyond the standard model physics. To pics include\, among others\, grand unification\, supersymmetry\, models o f extra dimensions and string models.\nTechnicalities will be avoided as m uch as possible.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a036 621 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a036621 END:VEVENT BEGIN:VEVENT SUMMARY:Physics beyond the Standard Model (2/5) DTSTART;VALUE=DATE-TIME:20040330T090000Z DTEND;VALUE=DATE-TIME:20040330T100000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a036622@cern.ch DESCRIPTION:I discuss several issues beyond the standard model physics. To pics include\, among others\, grand unification\, supersymmetry\, models o f extra dimensions and string models.\nTechnicalities will be avoided as m uch as possible.\n\nPlease note the transparencies file is a combined set for both lectures 2 and 3.\n\nhttp://indico.cern.ch/conferenceDisplay.py?c onfId=a036622 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a036622 END:VEVENT BEGIN:VEVENT SUMMARY:Physics beyond the Standard Model (3/5) DTSTART;VALUE=DATE-TIME:20040331T090000Z DTEND;VALUE=DATE-TIME:20040331T100000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a036623@cern.ch DESCRIPTION:I discuss several issues beyond the standard model physics. To pics include\, among others\, grand unification\, supersymmetry\, models o f extra dimensions and string models.\nTechnicalities will be avoided as m uch as possible.\n\nPlease note the transparencies file is a combined set for both lectures 2 and 3.\n\nhttp://indico.cern.ch/conferenceDisplay.py?c onfId=a036623 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a036623 END:VEVENT BEGIN:VEVENT SUMMARY:Physics beyond the Standard Model (4/5) DTSTART;VALUE=DATE-TIME:20040401T090000Z DTEND;VALUE=DATE-TIME:20040401T100000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a036624@cern.ch DESCRIPTION:I discuss several issues beyond the standard model physics. To pics include\, among others\, grand unification\, supersymmetry\, models o f extra dimensions and string models.\nTechnicalities will be avoided as m uch as possible.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a036 624 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a036624 END:VEVENT BEGIN:VEVENT SUMMARY:Physics beyond the Standard Model (5/5) DTSTART;VALUE=DATE-TIME:20040402T090000Z DTEND;VALUE=DATE-TIME:20040402T100000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a036625@cern.ch DESCRIPTION:I discuss several issues beyond the standard model physics. To pics include\, among others\, grand unification\, supersymmetry\, models o f extra dimensions and string models.\nTechnicalities will be avoided as m uch as possible.\n\nhttp://indico.cern.ch/conferenceDisplay.py?confId=a036 625 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a036625 END:VEVENT BEGIN:VEVENT SUMMARY:Electroweak Theory and the Standard Model (1/5) DTSTART;VALUE=DATE-TIME:20041206T100000Z DTEND;VALUE=DATE-TIME:20041206T110000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a042577@cern.ch DESCRIPTION:There is a natural splitting in four sectors of the theory of the ElectroWeak (EW) Interactions\, at pretty different levels of developm ent/test. Accordingly\, the 5 lectures are organized as follows\, with an eye to the future: Lecture 1: The basic structure of the theory\; Lecture 2: The gauge sector\; Lecture 3: The flavor sector\; Lecture 4: The neutr ino sector\; Lecture 5: The EW symmetry breaking sector.\n\nhttp://indico. cern.ch/conferenceDisplay.py?confId=a042577 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a042577 END:VEVENT BEGIN:VEVENT SUMMARY:Electroweak Theory and the Standard Model (2/5) DTSTART;VALUE=DATE-TIME:20041207T100000Z DTEND;VALUE=DATE-TIME:20041207T110000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a042578@cern.ch DESCRIPTION:There is a natural splitting in four sectors of the theory of the ElectroWeak (EW) Interactions\, at pretty different levels of developm ent/test. Accordingly\, the 5 lectures are organized as follows\, with an eye to the future: Lecture 1: The basic structure of the theory\; Lecture 2: The gauge sector\; Lecture 3: The flavor sector\; Lecture 4: The neutr ino sector\; Lecture 5: The EW symmetry breaking sector.\n\nhttp://indico. cern.ch/conferenceDisplay.py?confId=a042578 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a042578 END:VEVENT BEGIN:VEVENT SUMMARY:Electroweak Theory and the Standard Model (3/5) DTSTART;VALUE=DATE-TIME:20041208T100000Z DTEND;VALUE=DATE-TIME:20041208T110000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a042579@cern.ch DESCRIPTION:There is a natural splitting in four sectors of the theory of the ElectroWeak (EW) Interactions\, at pretty different levels of developm ent/test. Accordingly\, the 5 lectures are organized as follows\, with an eye to the future: Lecture 1: The basic structure of the theory\; Lecture 2: The gauge sector\; Lecture 3: The flavor sector\; Lecture 4: The neutr ino sector\; Lecture 5: The EW symmetry breaking sector.\n\nhttp://indico. cern.ch/conferenceDisplay.py?confId=a042579 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a042579 END:VEVENT BEGIN:VEVENT SUMMARY:Electroweak Theory and the Standard Model (4/5) DTSTART;VALUE=DATE-TIME:20041209T100000Z DTEND;VALUE=DATE-TIME:20041209T110000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a042580@cern.ch DESCRIPTION:There is a natural splitting in four sectors of the theory of the ElectroWeak (EW) Interactions\, at pretty different levels of developm ent/test. Accordingly\, the 5 lectures are organized as follows\, with an eye to the future: Lecture 1: The basic structure of the theory\; Lecture 2: The gauge sector\; Lecture 3: The flavor sector\; Lecture 4: The neutr ino sector\; Lecture 5: The EW symmetry breaking sector.\n\nhttp://indico. cern.ch/conferenceDisplay.py?confId=a042580 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a042580 END:VEVENT BEGIN:VEVENT SUMMARY:Electroweak Theory and the Standard Model (5/5) DTSTART;VALUE=DATE-TIME:20041210T100000Z DTEND;VALUE=DATE-TIME:20041210T110000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a042581@cern.ch DESCRIPTION:There is a natural splitting in four sectors of the theory of the ElectroWeak (EW) Interactions\, at pretty different levels of developm ent/test. Accordingly\, the 5 lectures are organized as follows\, with an eye to the future: Lecture 1: The basic structure of the theory\; Lecture 2: The gauge sector\; Lecture 3: The flavor sector\; Lecture 4: The neutr ino sector\; Lecture 5: The EW symmetry breaking sector.\n\nhttp://indico. cern.ch/conferenceDisplay.py?confId=a042581 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a042581 END:VEVENT BEGIN:VEVENT SUMMARY:Particle Detectors - Principles and Techniques (1/5) Introduction DTSTART;VALUE=DATE-TIME:20050411T090000Z DTEND;VALUE=DATE-TIME:20050411T100000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a042929@cern.ch DESCRIPTION:The lecture series presents an overview of the physical princi ples and basic techniques of particle detection\, applied to current and f uture high energy physics experiments. Illustrating examples\, chosen main ly from the field of collider experiments\, demonstrate the performance an d limitations of the various techniques.\nMain topics of the series are: i nteraction of particles and photons with matter\; particle tracking with g aseous and solid state devices\, including a discussion of radiation damag e and strategies for improved radiation hardness\; scintillation and photo n detection\; electromagnetic and hadronic calorimetry\; particle identifi cation using specific energy loss dE/dx\, time of flight\, Cherenkov light and transition radiation.\n\nhttp://indico.cern.ch/conferenceDisplay.py?c onfId=a042929 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a042929 END:VEVENT BEGIN:VEVENT SUMMARY:Particle Detectors - Principles and Techniques (2/5) Tracking DTSTART;VALUE=DATE-TIME:20050412T090000Z DTEND;VALUE=DATE-TIME:20050412T100000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a042930@cern.ch DESCRIPTION:The lecture series presents an overview of the physical princi ples and basic techniques of particle detection\, applied to current and f uture high energy physics experiments. Illustrating examples\, chosen main ly from the field of collider experiments\, demonstrate the performance an d limitations of the various techniques.\nMain topics of the series are: i nteraction of particles and photons with matter\; particle tracking with g aseous and solid state devices\, including a discussion of radiation damag e and strategies for improved radiation hardness\; scintillation and photo n detection\; electromagnetic and hadronic calorimetry\; particle identifi cation using specific energy loss dE/dx\, time of flight\, Cherenkov light and transition radiation.\n\nhttp://indico.cern.ch/conferenceDisplay.py?c onfId=a042930 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a042930 END:VEVENT BEGIN:VEVENT SUMMARY:Particle Detectors - Principles and Techniques (3/5) Scintillation and Photodetection DTSTART;VALUE=DATE-TIME:20050413T090000Z DTEND;VALUE=DATE-TIME:20050413T100000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a042931@cern.ch DESCRIPTION:The lecture series presents an overview of the physical princi ples and basic techniques of particle detection\, applied to current and f uture high energy physics experiments. Illustrating examples\, chosen main ly from the field of collider experiments\, demonstrate the performance an d limitations of the various techniques.\nMain topics of the series are: i nteraction of particles and photons with matter\; particle tracking with g aseous and solid state devices\, including a discussion of radiation damag e and strategies for improved radiation hardness\; scintillation and photo n detection\; electromagnetic and hadronic calorimetry\; particle identifi cation using specific energy loss dE/dx\, time of flight\, Cherenkov light and transition radiation.\n\nhttp://indico.cern.ch/conferenceDisplay.py?c onfId=a042931 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a042931 END:VEVENT BEGIN:VEVENT SUMMARY:Particle Detectors - Principles and Techniques (4/5) Calorimetry DTSTART;VALUE=DATE-TIME:20050414T090000Z DTEND;VALUE=DATE-TIME:20050414T100000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a042932@cern.ch DESCRIPTION:The lecture series presents an overview of the physical princi ples and basic techniques of particle detection\, applied to current and f uture high energy physics experiments. Illustrating examples\, chosen main ly from the field of collider experiments\, demonstrate the performance an d limitations of the various techniques.\nMain topics of the series are: i nteraction of particles and photons with matter\; particle tracking with g aseous and solid state devices\, including a discussion of radiation damag e and strategies for improved radiation hardness\; scintillation and photo n detection\; electromagnetic and hadronic calorimetry\; particle identifi cation using specific energy loss dE/dx\, time of flight\, Cherenkov light and transition radiation.\n\nhttp://indico.cern.ch/conferenceDisplay.py?c onfId=a042932 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a042932 END:VEVENT BEGIN:VEVENT SUMMARY:Particle Detectors - Principles and Techniques (5/5) Particle Iden tification and Detector Systems DTSTART;VALUE=DATE-TIME:20050415T090000Z DTEND;VALUE=DATE-TIME:20050415T100000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-a042933@cern.ch DESCRIPTION:The lecture series presents an overview of the physical princi ples and basic techniques of particle detection\, applied to current and f uture high energy physics experiments. Illustrating examples\, chosen main ly from the field of collider experiments\, demonstrate the performance an d limitations of the various techniques.\nMain topics of the series are: i nteraction of particles and photons with matter\; particle tracking with g aseous and solid state devices\, including a discussion of radiation damag e and strategies for improved radiation hardness\; scintillation and photo n detection\; electromagnetic and hadronic calorimetry\; particle identifi cation using specific energy loss dE/dx\, time of flight\, Cherenkov light and transition radiation.\n\nhttp://indico.cern.ch/conferenceDisplay.py?c onfId=a042933 LOCATION:CERN Main Auditorium URL:http://indico.cern.ch/conferenceDisplay.py?confId=a042933 END:VEVENT BEGIN:VEVENT SUMMARY:"Liquid Helium" Week DTSTART;VALUE=DATE-TIME:20100830T060000Z DTEND;VALUE=DATE-TIME:20100903T160000Z DTSTAMP;VALUE=DATE-TIME:20130523T042758Z UID:indico-event-90787@cern.ch DESCRIPTION:http://indico.cern.ch/conferenceDisplay.py?confId=90787 LOCATION:CERN 593-R-010 URL:http://indico.cern.ch/conferenceDisplay.py?confId=90787 END:VEVENT END:VCALENDAR